In 2002, the Institute of Electrical and Electronics Engineers (IEEE) released the 10 Gigabit Ethernet over fiber standard IEEE802.3ae. After that, based on optical fiber networks, 10 Gigabit data centers are constructed quickly and massively. On the other hand, because of the limitation of technology at that time and the bandwidth of copper cable, 10 Gigabit Ethernet 10GBASE-T technology couldn't be realized. However, the exploration of it was never stopped since the copper cable system has superior advantages in price and flexibility in short-range applications. Finally, in 2006, IEEE 802.3an standard was released to provide 10 Gbit/s speed connections over unshielded twisted pair copper cables, supporting distance up to 100 meters over Category 6A (Cat6A). And in 2012, Intel and Cisco launched a 10GBASE-T switch and network interface card (NIC), which indicates 10GBASE-T technology was applied to practice.

At normal incidence (zero order, λ3), the aberration is minimum and image is straight. But closer the images are from the grating, more stretched and curved are their images. This stretching can be severe, depends on the position of the image on the Rowland circle and hence of the observed wavelength. It results in both loss of signal and loss of resolution, especially in spectrograph mode when CCD detectors are used.

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QSFPTEK provides cost-effective and high-performance 10GBASE-T SFP+ transceivers, supporting links up to 30 meters over Cat6A or Cat7 at a low power consumption of less than 2.5W and the BER ( Bit Error Rate) is below 10^-12. QSFPTEK 10G copper transceivers are widely compatible with almost all original equipment manufacturers 10GBASE-T switches, NICs, and servers, like Cisco, Juniper, Arista, Intel, HPE, etc. Welcome to consult via sales@qsfptek.com.

An optical system with astigmatism is one where rays that propagate in two perpendicular planes have different focal points.

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A VLS grating is one whose grooves, when projected onto the tangent plane, form a set of straight parallel lines whose spacing varies from groove to groove. Varying the groove spacing across the surface of the grating moves the tangential focal curve, while keeping the grooves straight and parallel keeps the sagittal focal curve fixed. It corrects for spherical aberration associated with conventional spherical gratings. The VLS technique can also be applied on toroidal grating for an optimum correction.

Auto-negotiate and Backward Compatible. 10GBASE-T offers immense flexibility with its auto-negotiate function. It supports backward compatibility and interoperation with existing 1Gbps or 100Mbps Ethernet networks. This means you could gradually increase expenditure during upgrading your data center to 10 Gbps instead of upgrading all servers and switches to 10Gb/s on a large scale at once.

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The above introduction has told the max transmission distance of the 10GBASE-T copper transceiver is 100 meters over Cat6A. How about Cat5e, Cat6, or Cat7? Can they work on 10GBASE-T SFP+ to achieve a speed of 10Gbps? Which one is more suitable for 10G networks?

Chromatic aberration is a type of distortion in which the lens fails to focus all colors on the same convergence point, due to the dispersion of the lens (different refractive index of the lens for different wavelengths of light).

Low Cost. Compared to the 10G SFP+ fiber system, the SFP+ copper system offers a lower cost for the copper transmission media is much cheaper than fiber media.

10GBASE-T SFP+ transceiver is also known as the 10G copper RJ45 transceiver with interfacing an RJ45 port. Through this RJ45 port, 10 Gigabit differential signals are input into the SFP+ copper transceiver over the Cat6A cable. And then the inputted signals will experience filter and shaping to ensure the signals are complete and clean when inputting to the physical layer (PHY). Finally, the signals output after data decoding in PHY. The working diagram of the SFP+ RJ45 copper transceiver is as follows.

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The optimization of the image correction of gratings can be calculated for a better image quality on the optical axis of the instrument (monochromator layout) or on a focal plane (spectrograph layout). In the last case, the optimization enlarges the focal plane, the grating of the spectrograph works in fixed position and the wavelength range selection is achieved by sliding the detector in the focal plane of the instrument. The correction is excellent in both cases.

The design of VUV instruments suffers from the constraints of VUV optical materials. Transmission through bulk materials is limited to λ < 105 nm, the short wavelength transmission is limited of LiF or λ < 115 nm for MgF2. Reflective configuration is used in a VUV optical layout. However, reflectance from metal surfaces also decreases at short wavelengths. Several coating materials are introduced to increase reflectivity, such as Al, Os, Pt, Au, Rh and Ir. Above 120 nm, the main broadband reflector for VUV wavelengths is Al with MgF2 coating, having a normal incidence reflectivity of up to 90% under certain conditions. Os, Pt, Au, and Ir have a reflectance of about 60% from 5-200 nm in grazing configuration.

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10GBASE-T is a local area network (LAN) connection technology applied in 10 Gigabit Ethernet. Using unshielded twisted pair (UTP) copper cable as transmission medium, 10GBASE-T SFP+ transceiver supports a data rate of 10Gbps/s at a link distance up to 100 meters over Cat6A twisted copper cable.

Same as Cat6A, Cat7 supports 10Gbps at a distance of up to 100 meters. However, since using a double-layer shielding, the wire diameter Cat7 is much larger than Cat6A. So Cat7 takes up more space and also brings inconvenience to cabling. Moreover, the connector of Cat7 is special GG45 or TERA instead of common RJ45, thus the compatibility is not as good as Cat6A.

Copper twisted-pair-based Ethernet technology standard was first released in 1990, which defined 10BASE-T over twisted pair at the speed of 10 Mbit/s. After two decades, the twisted pair Ethernet has evolved from 10BASE-T to 100BASE-T to 1000BASE-T and now to 10GBASE-T. Compared to its predecessors, 10GBASE-T uses more complicated pulse-amplitude modulation of PAM-16 and Tomlinson-Harashima precoding (THP) to achieve 10 Gbps throughput. The technical differences between 10GBASE-T, 1000BASE-T, and 100BASE-T are shown in the following table.

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Two basic types of spectrographs and monochromators are used in the VUV: normal incidence instruments a better design for 100-400 nm, and grazing incidence instruments for 2-100 nm.

Unfortunately, gratings suffer from the aberrations of concave mirrors and others due to their diffraction capabilities. Working in the Rowland conditions definitively limits the imaging quality of the instruments. The major aberration here is astigmatism. This aberration can be tolerated with a monochromator since only horizontal focusing is required to separate the wavelengths of spectrum.

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An optical aberration is a departure of the performance of an optical system from the predictions of paraxial optics. In the existence of an optical aberration, light from one point of an object does not converge into (or does not diverge from) a single point after transmission through the system. Optical aberrations fall into two classes: monochromatic and chromatic.

Distortion is the most easily recognized aberration as it deforms the image as whole. It arises from the unequal magnification of the peripheral part of a lens (or a mirror) from that of its central part. In “barrel distortion,” image magnification decreases with distance from the optical axis. In “pincushion distortion,” image magnification increases with the distance from the optical axis.

With the advantages of low cost and flexibility, the copper twisted-pair-based 10GBASE-T cabling system has quickly seized part of the market previously occupied by 10 Gigabit optical fibers. However, there are also challenges for it.

As for Cat5A, it is disappointing to note that 10G copper transceivers can't properly work over Cat5A at a speed of 10Gbps. If you have to connect Cat5A with the SFP+ copper Rj45 transceiver, the transceiver may auto-negotiate to 1000Mbps. However, Cat6A is cheap, so why not directly upgrade your Cat5A to Cat6 to enjoy better network performance?

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The realization of a real VUV monograph has to be done without a toroidal grating. The Plane Grating Spectrograph (PGS) configuration is one of the best choices. The PGS layout operates with a toroid mirror and a plane grating working at a grazing angle. It also has the advantage of being more affordable grating as they have a plane design.

The spectroscopic images can be improved by using toroidal gratings. A toroidal grating is a form of an elliptic paraboloid with different vertical and horizontal focal distances. It reduces the stretching and the curvature of astigmatism.

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To increase the transmission data rate to 10 Gigabit, Cat6A cables are required to reach 500 MHz frequency. The transmission performance is sensitive to external crosstalk in such a high frequency. What is external crosstalk? In equipment rooms or offices, various wires are generally tied up and placed in a slot. One of the wire pairs will be disturbed by others in the same bundle of wires. That is external crosstalk. The following picture shows the crosstalk of one cable caused by surrounding cables.

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A master grating is an original unit recorded as a unique piece. A master grating can be utilized as the “mother” of multiples copies, called replicas.

Monochromatic aberrations are caused by the geometry of the lens and occur both when light is reflected and when it is refracted. Monochromatic aberrations include spherical aberration, coma, astigmatism, and field curvature and image distortion.

S: Spot source (or slit of the instrument) λ3: Zero order position λ1, λ2: Dispersed wavelength positions λ1> λ2 i: incidence angle r: reflectance angle

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Most of the time, VUV monochromators are preferred when equipped with master gratings. But unfortunately, such gratings are extremely expensive and have a long delivery time.

Aberration leads to blurring of the image produced by an image-forming optical system. Makers of optical instruments need to correct optical systems to compensate for aberration.

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Compared to fiber-based SFP+ transceivers, 10GBASE-T transceivers require a higher power consumption. The max power consumption of a 10GBASE SR SFP+ optical transceiver is only 0.8W, while the 10G copper transceiver is 2.5W. So it may appear to be cheaper on a copper cable basis, but the power consumption needed to support 10G copper RJ45 over Cat6A is tremendous compared to Optics.

Some aberration affects the images due to off axis rays. The image of a spot looks like several cylinders not centered, like an image of a “comet”, where its name comes from.

A Rowland demonstrated that the dispersed spectrum of an illuminated point lying on a circle is focused on this circle, if the following setup is respected (see figure). A lot of VUV monochromators use this design.

In order to limit the number of reflections onto optics, concave gratings are often used as single element in VUV spectrometers.

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Spherically shaped lenses and mirrors share this problem. Parallel light rays that pass through the central region focus farther away than those that pass through the edges. The result is many focal points, which produces a blurry image.